Dimmer
Astronomy C
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Re: Astronomy C
Lower Merion 2017
Subtitled: Revenge of the Non-Harriton
Placement Record:
Code: Islip | Conestoga | Tiger | Regionals | States
Out of: 61 | 42 | 36 | 37 | 36
Chemistry Lab: 9 | - | - | 4 | 4
Astronomy: 14 | - | 5 | 10 | 3
Material Science: 12 | 19 | 9 | 5 | 9
Optics: 14 | 7 | 3 | 4 | 2
Subtitled: Revenge of the Non-Harriton
Placement Record:
Code: Islip | Conestoga | Tiger | Regionals | States
Out of: 61 | 42 | 36 | 37 | 36
Chemistry Lab: 9 | - | - | 4 | 4
Astronomy: 14 | - | 5 | 10 | 3
Material Science: 12 | 19 | 9 | 5 | 9
Optics: 14 | 7 | 3 | 4 | 2
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Re: Astronomy C
I messed up, you were correct, this is called the luminosity decline rate relation.Unome wrote:dimmer drops faster?
Last edited by jonboyage on Thu Feb 02, 2017 9:09 am, edited 2 times in total.
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Rustin '19
UPenn '23
Rustin '19
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Re: Astronomy C
jonboyage wrote:Unome wrote:dimmer drops faster?I have read in the past that the brighter ones drop faster
[quote="Wikipedia - Phillips relationship"]They found that the faster the supernova faded from maximum light, the fainter its peak magnitude was[/quote]
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Re: Astronomy C
Yeah you were right sorry, I checked online right after I posted just to make sure and I found that the dimmer ones drop faster.
Do you want to ask the next one?
Do you want to ask the next one?
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Re: Astronomy C
jonboyage wrote:Yeah you were right sorry, I checked online right after I posted just to make sure and I found that the dimmer ones drop faster.
Do you want to ask the next one?
A type Ia supernova is discovered in a distant galaxy. Its maximum apparent magnitude is measured at 18.4. After monitoring the supernova for 15 days, the B band magnitude drops by 1.2. 1. What is the theoretical absolute luminosity of a type Ia supernova originating from a single progenitor? 2. Calculate the distance to the supernova based on this theoretical absolute magnitude. 3. Determine the speed at which the galaxy containing the supernova is receding. Use a Hubble constant of 70 km^-1*Mpc^-1 4. Based on the luminosity decline, determine the actual absolute magnitude of the supernova. 5. Recalculate the distance and recessional velocity based on the actual absolute magnitude.
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Re: Astronomy C
Unome wrote:jonboyage wrote:Yeah you were right sorry, I checked online right after I posted just to make sure and I found that the dimmer ones drop faster.
Do you want to ask the next one?A type Ia supernova is discovered in a distant galaxy. Its maximum apparent magnitude is measured at 18.4. After monitoring the supernova for 15 days, the B band magnitude drops by 1.2. 1. What is the theoretical absolute luminosity of a type Ia supernova originating from a single progenitor? 2. Calculate the distance to the supernova based on this theoretical absolute magnitude. 3. Determine the speed at which the galaxy containing the supernova is receding. Use a Hubble constant of 70 km^-1*Mpc^-1 4. Based on the luminosity decline, determine the actual absolute magnitude of the supernova. 5. Recalculate the distance and recessional velocity based on the actual absolute magnitude.
1. -19.3 2. 346.7mpc 3. 24271.6km/s 4. -18.4884 5. 238.6mpc; 16702.4km/s
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Re: Astronomy C
Sorry for jumping in but I have a question. How did you calculate the absolute magnitude in question 4? I've looked up luminosity decline rate and a couple other things and I haven't been able to find anything. Thanks in advance.jonboyage wrote:Unome wrote:jonboyage wrote:Yeah you were right sorry, I checked online right after I posted just to make sure and I found that the dimmer ones drop faster.
Do you want to ask the next one?A type Ia supernova is discovered in a distant galaxy. Its maximum apparent magnitude is measured at 18.4. After monitoring the supernova for 15 days, the B band magnitude drops by 1.2. 1. What is the theoretical absolute luminosity of a type Ia supernova originating from a single progenitor? 2. Calculate the distance to the supernova based on this theoretical absolute magnitude. 3. Determine the speed at which the galaxy containing the supernova is receding. Use a Hubble constant of 70 km^-1*Mpc^-1 4. Based on the luminosity decline, determine the actual absolute magnitude of the supernova. 5. Recalculate the distance and recessional velocity based on the actual absolute magnitude.1. -19.3 2. 346.7mpc 3. 24271.6km/s 4. -18.4884 5. 238.6mpc; 16702.4km/s
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Re: Astronomy C
I simply used the formula for the Philips relationship which you can easily find the Wikipedia page for. The formula is this: M_max(B) = -21.726 + 2.698Δm_15(B). This formula is very specific to the scenario given here: after 15 days, the B-band magnitude drops by 1.2. Hope that helps!Bob_117 wrote:Sorry for jumping in but I have a question. How did you calculate the absolute magnitude in question 4? I've looked up luminosity decline rate and a couple other things and I haven't been able to find anything. Thanks in advance.jonboyage wrote:Unome wrote:A type Ia supernova is discovered in a distant galaxy. Its maximum apparent magnitude is measured at 18.4. After monitoring the supernova for 15 days, the B band magnitude drops by 1.2. 1. What is the theoretical absolute luminosity of a type Ia supernova originating from a single progenitor? 2. Calculate the distance to the supernova based on this theoretical absolute magnitude. 3. Determine the speed at which the galaxy containing the supernova is receding. Use a Hubble constant of 70 km^-1*Mpc^-1 4. Based on the luminosity decline, determine the actual absolute magnitude of the supernova. 5. Recalculate the distance and recessional velocity based on the actual absolute magnitude.1. -19.3 2. 346.7mpc 3. 24271.6km/s 4. -18.4884 5. 238.6mpc; 16702.4km/s
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Re: Astronomy C
Sorry, forgot about this during prep for regionals. Correct, your turn.jonboyage wrote:I simply used the formula for the Philips relationship which you can easily find the Wikipedia page for. The formula is this: M_max(B) = -21.726 + 2.698Δm_15(B). This formula is very specific to the scenario given here: after 15 days, the B-band magnitude drops by 1.2. Hope that helps!Bob_117 wrote:Sorry for jumping in but I have a question. How did you calculate the absolute magnitude in question 4? I've looked up luminosity decline rate and a couple other things and I haven't been able to find anything. Thanks in advance.jonboyage wrote:1. -19.3 2. 346.7mpc 3. 24271.6km/s 4. -18.4884 5. 238.6mpc; 16702.4km/s
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Re: Astronomy C
I'll pick this up then.
Some standard math:
Star A has a temperature of 6400 K.
1. Calculate its peak wavelength in nm.
2. The real wavelength is measured to be 480 nm. What is the recessional velocity of the star in m/s?
3. Is this number reasonable?
4. Star A is part of system AB, which has an apparent magnitude of 6.4 and an absolute magnitude of 1.99. Star B has a luminosity of 5.0 solar luminosities. What is the radius of star A in solar radii?
5. How far away is system AB in parsecs, light years, AU, and meters?
Some standard math:
Star A has a temperature of 6400 K.
1. Calculate its peak wavelength in nm.
2. The real wavelength is measured to be 480 nm. What is the recessional velocity of the star in m/s?
3. Is this number reasonable?
4. Star A is part of system AB, which has an apparent magnitude of 6.4 and an absolute magnitude of 1.99. Star B has a luminosity of 5.0 solar luminosities. What is the radius of star A in solar radii?
5. How far away is system AB in parsecs, light years, AU, and meters?
Ladue Science Olympiad (2014ish-2017)
A wild goose flies over a pond, leaving behind a voice in the wind.
A man passes through this world, leaving behind a name.
A wild goose flies over a pond, leaving behind a voice in the wind.
A man passes through this world, leaving behind a name.